{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:DNJF63BZ7H6OIJAG26KKGLFMMK","short_pith_number":"pith:DNJF63BZ","schema_version":"1.0","canonical_sha256":"1b525f6c39f9fce42406d794a32cac62a77cd3b8d30c495ed491dde411ef32fe","source":{"kind":"arxiv","id":"1107.3585","version":3},"attestation_state":"computed","paper":{"title":"Model-Independent Comparisons of Pulsar Timings to Scalar-Tensor Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"C. P. Burgess, M. W. Horbatsch","submitted_at":"2011-07-18T21:50:34Z","abstract_excerpt":"Observations of pulsar timing provide strong constraints on scalar-tensor theories of gravity, but these constraints are traditionally quoted as limits on the microscopic parameters (like the Brans-Dicke coupling, for example) that govern the strength of scalar-matter couplings at the particle level in particular models. Here we present fits to timing data for several pulsars directly in terms of the phenomenological couplings (masses, scalar charges, moment of inertia sensitivities and so on) of the stars involved, rather than to the more microscopic parameters of a specific model. For instan"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1107.3585","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2011-07-18T21:50:34Z","cross_cats_sorted":["astro-ph.GA","hep-ph","hep-th"],"title_canon_sha256":"711dfcda8757d6b33d1fa7ee9bfd1d3b665654f67e8d5445acc86fef0ec29f13","abstract_canon_sha256":"c0e203a65622922bedf907b21b9956feb210ccaedba12c65c2240af6b9abb78c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:15.198837Z","signature_b64":"GzmdYPy4yfjOnOr19LBWA4kfwFv47o7jt4iG3YOytPFsxM29paPsanKLPrbfQUahmQnLQATQ+eT1BBg4s5XFBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b525f6c39f9fce42406d794a32cac62a77cd3b8d30c495ed491dde411ef32fe","last_reissued_at":"2026-05-18T02:01:15.198343Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:15.198343Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Model-Independent Comparisons of Pulsar Timings to Scalar-Tensor Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"C. P. Burgess, M. W. Horbatsch","submitted_at":"2011-07-18T21:50:34Z","abstract_excerpt":"Observations of pulsar timing provide strong constraints on scalar-tensor theories of gravity, but these constraints are traditionally quoted as limits on the microscopic parameters (like the Brans-Dicke coupling, for example) that govern the strength of scalar-matter couplings at the particle level in particular models. Here we present fits to timing data for several pulsars directly in terms of the phenomenological couplings (masses, scalar charges, moment of inertia sensitivities and so on) of the stars involved, rather than to the more microscopic parameters of a specific model. For instan"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.3585","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1107.3585","created_at":"2026-05-18T02:01:15.198414+00:00"},{"alias_kind":"arxiv_version","alias_value":"1107.3585v3","created_at":"2026-05-18T02:01:15.198414+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.3585","created_at":"2026-05-18T02:01:15.198414+00:00"},{"alias_kind":"pith_short_12","alias_value":"DNJF63BZ7H6O","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_16","alias_value":"DNJF63BZ7H6OIJAG","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_8","alias_value":"DNJF63BZ","created_at":"2026-05-18T12:26:26.731475+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK","json":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK.json","graph_json":"https://pith.science/api/pith-number/DNJF63BZ7H6OIJAG26KKGLFMMK/graph.json","events_json":"https://pith.science/api/pith-number/DNJF63BZ7H6OIJAG26KKGLFMMK/events.json","paper":"https://pith.science/paper/DNJF63BZ"},"agent_actions":{"view_html":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK","download_json":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK.json","view_paper":"https://pith.science/paper/DNJF63BZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1107.3585&json=true","fetch_graph":"https://pith.science/api/pith-number/DNJF63BZ7H6OIJAG26KKGLFMMK/graph.json","fetch_events":"https://pith.science/api/pith-number/DNJF63BZ7H6OIJAG26KKGLFMMK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK/action/storage_attestation","attest_author":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK/action/author_attestation","sign_citation":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK/action/citation_signature","submit_replication":"https://pith.science/pith/DNJF63BZ7H6OIJAG26KKGLFMMK/action/replication_record"}},"created_at":"2026-05-18T02:01:15.198414+00:00","updated_at":"2026-05-18T02:01:15.198414+00:00"}